|
Depth
|
Offset (m)
|
||
|---|---|---|---|
|
Logging
|
Core (mbsf)
|
Core (mcd)
|
|
| 116.82 | 110.80 | 105.30 | 6.02 |
| 123.78 | 118.78 | 113.28 | 5.00 |
| 130.52 | 124.48 | 118.98 | 6.04 |
| 133.54 | 127.62 | 122.12 | 5.92 |
| 139.82 | 134.82 | 129.32 | 5.00 |
| 147.94 | 143.28 | 137.78 | 4.66 |
| 152.10 | 148.04 | 142.54 | 4.06 |
| 156.32 | 150.76 | 145.26 | 5.56 |
| 158.82 | 153.10 | 147.60 | 5.72 |
| 161.02 | 156.12 | 150.62 | 4.90 |
| 164.20 | 159.62 | 154.12 | 4.58 |
| 169.14 | 163.76 | 158.26 | 5.38 |
| 174.74 | 169.70 | 164.20 | 5.04 |
| 175.94 | 171.50 | 166.00 | 4.44 |
| 186.48 | 182.52 | 177.02 | 3.96 |
| 190.46 | 187.16 | 181.66 | 3.30 |
| 200.44 | 196.82 | 191.32 | 3.62 |
| 202.12 | 197.42 | 191.92 | 4.70 |
| 204.96 | 200.42 | 194.92 | 4.54 |
| 220.26 | 214.84 | 209.34 | 5.42 |
| 221.08 | 215.50 | 210.00 | 5.58 |
| 240.84 | 235.86 | 230.36 | 4.98 |
| 255.96 | 250.44 | 244.94 | 5.52 |
| 268.88 | 263.64 | 258.14 | 5.24 |
| 282.66 | 277.08 | 271.58 | 5.58 |
| 312.22 | 306.80 | 301.30 | 5.42 |
| 320.84 | 315.26 | 309.76 | 5.58 |
| 327.12 | 320.90 | 315.40 | 6.22 |
| 356.98 | 351.30 | 345.80 | 5.68 |
| 362.16 | 356.72 | 351.22 | 5.44 |
| 370.12 | 365.64 | 360.14 | 4.48 |
| 374.02 | 368.84 | 363.34 | 5.18 |
| 380.88 | 376.50 | 371.00 | 4.38 |
| 400.12 | 395.02 | 389.52 | 5.10 |
| 404.10 | 399.70 | 394.20 | 4.40* |
| 418.30 | 412.76 | 407.26 | 5.54 |
| 423.22 | 418.28 | 412.78 | 4.94 |
| 465.06 | 459.86 | 454.36 | 5.20 |
| 478.98 | 474.14 | 468.64 | 4.84 |
| 492.42 | 485.74 | 480.24 | 6.68* |
Notes: Correlation of whole-core susceptibility with susceptibility measured on the second run of the GHMT logging tool was completed using version 1.2 of the program AnalySeries (Paillard et al., 1996). Linear interpolation is used between tie points to convert from one depth scale to another. * = these tie points are secondary adjustments based on comparing the paleomagnetic inclination data to the remanent anomaly calculated from the second logging run of the GHMT. Offset = logging depth - mbsf depth.